Twenty Halpa and R images of galaxies in the NRGb032 group, taken at Kitt Peak National Observatory, are processed and analyzed to determine information about star formation in the group environment; namely where stars are forming and their density of formation. We find that the star formation rates of the NRGb032 group were similar to the galaxies in the Virgo cluster: star formation rates were depressed overall, typical of isolated galaxies in the inner regions and missing in the outer regions. These results will be compared to results in clusters, results obtained by previous students, and results of other member of the Undergraduate ALFALFA Team.
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